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1
The JWST-SUSPENSE Ultradeep Spectroscopic Program: Survey Overview and Star Formation Histories of Quiescent Galaxies at 1 < z < 3
Published 2024-01-01Subjects: Get full text
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2
JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe
Published 2025-01-01Subjects: “…Galaxy formation…”
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3
Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at 0.7 ≲ z ≲ 9.3 with NIRSpec High-resolution Spectroscopy
Published 2025-01-01Subjects: “…Galaxy formation…”
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4
UNCOVER: The Rest-ultraviolet to Near-infrared Multiwavelength Structures and Dust Distributions of Submillimeter-detected Galaxies in A2744
Published 2025-01-01Subjects: “…Galaxy formation…”
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5
CEERS: Increasing Scatter along the Star-forming Main Sequence Indicates Early Galaxies Form in Bursts
Published 2025-01-01Subjects: Get full text
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6
Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows
Published 2025-01-01Subjects: Get full text
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7
Cluster Candidates with Massive Quiescent Galaxies at z ∼ 2
Published 2025-01-01Subjects: Get full text
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8
The Prevalence of Star-forming Clumps as a Function of Environmental Overdensity in Local Galaxies
Published 2025-01-01Subjects: Get full text
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9
Blowing Out the Candle: How to Quench Galaxies at High Redshift—An Ensemble of Rapid Starbursts, AGN Feedback, and Environment
Published 2025-01-01Subjects: Get full text
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10
Physical Pathways for JWST-observed Supermassive Black Holes in the Early Universe
Published 2025-01-01Subjects: Get full text
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11
Investigating the Lower Limit of Metallicity for the Galactic Thin Disk
Published 2025-01-01Subjects: Get full text
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12
Pearls on a String: Dark and Bright Galaxies on a Strikingly Straight and Narrow Filament
Published 2025-01-01Subjects: Get full text
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13
The Rapid Formation of the Metal-poor Milky Way
Published 2025-01-01Subjects: Get full text
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14
Improving H2RG Performance in SPHEREx Brassboard Model
Published 2025-01-01“…Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer is an upcoming NASA satellite mission to study the physics of inflation, the history of galaxy formation, and the abundance of biogenic ices in the Milky Way, obtaining the first all-sky spectroscopic survey at infrared wavelengths 0.75–5.0 μ m. …”
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15
Galaxy Evolution in a Pilot Survey up to z=1 and CDM Halos
Published 2011-01-01“…Therefore at redshifts z⩽1 galaxy formation is downsizing both in luminosity and number density. …”
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16
Cosmic Reionization on Computers: The Evolution of the Ionizing Background and Mean Free Path
Published 2025-01-01“…In this study, we utilize the Cosmic Reionization on Computers (CROC) simulations, which have both sufficient spatial resolution to resolve galaxy formation and LLSs alongside a fully coupled radiative transfer, to simulate the reionization processes. …”
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17
Ejective Feedback as a Quenching Mechanism in the First 1.5 Billion Years of the Universe: Detection of Neutral Gas Outflow in a z = 4 Recently Quenched Galaxy
Published 2025-01-01“…The confirmation of massive quiescent galaxies emerging within the first billion years of the Universe poses intriguing questions about the mechanisms of galaxy formation. There must be highly efficient processes at work to shut down star formation in galaxies at cosmic dawn. …”
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18
The Theory of Resonant Cosmic Ray–driven Instabilities—Growth and Saturation of Single Modes
Published 2025-01-01“…Cosmic-ray (CR) feedback is critical for galaxy formation as CRs drive galactic winds, regularize star formation in galaxies, and escape from active galactic nuclei to heat the cooling cores of galaxy clusters. …”
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19
Quantifying Baryonic Feedback on the Warm–Hot Circumgalactic Medium in CAMELS Simulations
Published 2025-01-01“…The baryonic physics shaping galaxy formation and evolution are complex, spanning a vast range of scales and making them challenging to model. …”
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20
Deep Learning for Identification and Characterization of Ca ii Absorption Lines: A Multitask Convolutional Neural Network Approach
Published 2025-01-01“…Quasar absorption lines are a powerful tool for studying the Universe, enabling us to probe distant gas, dust, and galaxy formation and evolution. However, detecting these lines, particularly Ca ii absorption lines, is a time-consuming and laborious process. …”
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